ASCA studies of the hot gas in clusters of galaxies.

Details ASCA studies of the hot gas in clusters of galaxies. ASCA studies of the hot gas in clusters of galaxies.

Feb 1996

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1996rftu.proc..605o&link_type=abstract

International Conference on X-ray Astronomy and Astrophysics: Röntgenstrahlung from the Universe, p. 605 - 606

Astronomy and Astrophysics

Astrophysics

1

Iron: Clusters Of Galaxies, Iron: Galaxy Groups, X Rays: Clusters Of Galaxies, X Rays: Galaxy Groups, Metal Abundances: Galaxy Groups, Metal Abundances: Clusters Of Galaxies

Scientific paper

The abundance measurement in the hot plasma in clusters of galaxies and in poor groups of galaxies with ASCA are summarized. Clusters show narrow concentration of the iron abundance around 0.35 solar for different temperatures of the intracluster medium for 2-7 keV. The analysis including the effect of the XRT show good isothermality of the gas in 3A 0336+098. Unusually low metal abundance (<0.1 solar) has been observed from poor groups, and possible causes are discussed.

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